A catalogue of galaxies behind the southern Milky Way ? II. The Crux and Great Attractor regions (l approximate to 289 degrees to 338 degrees)

In this second paper of the catalogue series of galaxies behind the souther n Milky Way, we report on the deep optical galaxy search in the Crux region (289 degrees less than or equal to l less than or equal to 318 degrees and -10 degrees less than or equal to b less than or equal to 10 degrees) and the Great Attractor region (316 degrees less than or equal to l less than o r equal to 338 degrees and -10 degrees less than or equal to b less than or equal to 10 degrees). The galaxy catalogues are presented, a brief descrip tion of the galaxy search given, as well as a discussion on the distributio n and characteristics of the uncovered galaxies. A total of 8182 galaxies w ith major diameters D greater than or similar to 0.'2 were identified in th is similar to 850 square degree area: 3759 galaxies in the Crux region and 4423 galaxies in the Great Attractor region. Of the 8182 galaxies, 229 (2.8 %) were catalogued before in the optical (3 in radio) and 251 galaxies have a reliable (159), or likely (92) cross-identification in the IRAS Point So urce Catalogue (3.1%). A number of prominent overdensities and filaments of galaxies are identified. They are not correlated with the Galactic foregro und extinction and hence indicative of extragalactic large-scale structures . Redshifts obtained at the South African Astronomical Observatory (SAAO) f or 518 of the newly catalogued galaxies in the Crux and Great Attractor reg ions (Fairall et al. 1998; Woudt et al. 1999) confirm distinct voids and cl usters in the area here surveyed. With this optical galaxy search, we have reduced the width of the optical "Zone of Avoidance" for galaxies with exti nction-corrected diameters larger than 1.3 arcmin from extinction levels A( B) greater than or equal to 1.(m)0 to A(B) greater than or equal to 3.(m)0: the remaining optical Zone of Avoidance is now limited by \b\ less than or similar to 3 degrees (see Fig. 16).